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| 20240204 - Filament data for 08 UTC |
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Available data for 20240204: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 725 1814 (N42E43 L= 92) 1376 122 1 ( 674/1764- 771/1852) -14.0 E52-E36 N37-N45
2 987 1682 (N35E15 L=121) 262 36 1 ( 967/1662-1011/1704) -14.0 E16-E12 N33-N36
3 1144 1663 (N36E03 L=132) 289 33 1 (1124/1635-1158/1690) -76.0 E04-E01 N34-N38
4 476 1643 (N26E52 L= 83) 598 79 2 ( 441/1606- 508/1673) -21.8 E57-E47 N23-N27
5 1519 1639 (N43W28 L=163) 568 50 1 (1499/1606-1548/1667) 50.2 W25-W31 N39-N45
6 1642 1329 (N23W37 L=172) 1183 302 0 (1550/1224-1711/1457) -42.7 W29-W42 N17-N29
7 1869 1329 (N29W63 L=198) 841 90 0 (1830/1305-1906/1352) 12.1 W56-W70 N26-N30
8 583 1060 (S10E28 L=107) 337 77 1 ( 543/1036- 621/1085) 21.8 E30-E25 S11-S08
9 111 1002 (S17E74 L= 61) 4361 168 6 ( 76/ 910- 164/1072) 60.9 E85-E64 S21-S12
10 1569 1004 (N02W34 L=169) 320 78 1 (1526/ 985-1601/1033) 36.9 W31-W35 N00-N03
11 1843 955 (N05W58 L=193) 519 80 1 (1817/ 909-1862/ 988) -33.7 W54-W61 N02-N06
12 362 900 (S22E43 L= 92) 437 109 1 ( 309/ 867- 404/ 932) -12.5 E48-E39 S23-S19
13 851 881 (S17E08 L=127) 298 61 1 ( 813/ 860- 879/ 907) 36.9 E10-E06 S18-S15
14 1557 881 (S06W35 L=170) 224 46 0 (1533/ 859-1581/ 906) -26.6 W33-W37 S06-S04
15 1493 686 (S18W36 L=171) 353 73 0 (1457/ 656-1524/ 719) 53.1 W34-W37 S20-S15
16 1533 582 (S23W43 L=178) 532 80 1 (1497/ 558-1580/ 610) -7.1 W39-W47 S24-S22
17 580 432 (S51E28 L=107) 637 73 1 ( 553/ 388- 603/ 469) -63.4 E30-E26 S54-S48
18 1504 448 (S32W48 L=183) 392 80 0 (1474/ 412-1528/ 469) -63.4 W44-W50 S34-S30
19 1099 329 (S49W23 L=158) 578 167 0 (1024/ 292-1140/ 382) 49.4 W17-W25 S53-S44
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Download FITS filament maps as tar archive
» All Filament Data of 20240204 ...
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The tar archive contains filament maps for all processed Hα images
with at least quality=1.
The maps contain the values 0 and 1, where 1 is the position of a detected filament.
The header in the FITS files is mostly taken from the corresponding Hα file,
so it should be compatible with standard solar software routines.
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